Research

My PhD project is focused on making new detections of the Yarkovsky–O’Keefe–Radzievskii–Paddack (YORP) effect. The YORP effect is a small torque experienced by small bodies in the Solar System, caused by the  absorption and anisotropic re-emission of thermal radiation from the Sun. 

YORP can have a profound influence on the evolution of asteroids, through modification of their rotation rates and spin axis orientations. It contributes to the replenishment of the near-Earth asteroid population, forms binary systems, aligns the spin-axis orientation of asteroid families  and can trigger rotational fission or tumbling. 

There are relatively few published detections of the YORP effect. My research is focused on making new detections with a long-term optical observing campaign, which focuses on a small sample of near-Earth asteroids.

In order to detect the YORP effect, a physical model of the asteroid must be developed to describe its shape and spin-state.  This model is used to generate synthetic lightcurves, against which observations can be compared. YORP can then be detected through any rotational phase offset between observations and a constant-period model.

I develop asteroid models using a combination of optical and radar data. As such, my research interests are more broadly focused on the observation and characterisation of small bodies in the Solar System. 

Selected Publications

Conferences